In statistics, the standard score is the number of standard deviations by which the value of a raw score (i.e., an observed value or data point) is above or below the mean value of what is being observed or measured. Raw scores above the mean have positive standard scores, while those below the mean have negative standard scores.
It is calculated by subtracting the population mean from an individual raw score and then dividing the difference by the population standard deviation. This process of converting a raw score into a standard score is called standardizing or normalizing (however, "normalizing" can refer to many types of ratios; see Normalization for more).
Standard scores are most commonly called z-scores; the two terms may be used interchangeably, as they are in this article. Other equivalent terms in use include z-value, z-statistic, normal score, standardized variable and pull in high energy physics.[1][2]
Computing a z-score requires knowledge of the mean and standard deviation of the complete population to which a data point belongs; if one only has a sample of observations from the population, then the analogous computation using the sample mean and sample standard deviation yields the t-statistic.
- ^ Mulders, Martijn; Zanderighi, Giulia, eds. (2017). 2015 European School of High-Energy Physics: Bansko, Bulgaria 02 - 15 Sep 2015. CERN Yellow Reports: School Proceedings. Geneva: CERN. ISBN 978-92-9083-472-4.
- ^ Gross, Eilam (2017-11-06). "Practical Statistics for High Energy Physics". CERN Yellow Reports: School Proceedings. 4/2017: 165–186. doi:10.23730/CYRSP-2017-004.165.